A Dark Energy Model with Higher Derivative and Cosmological Evolution

被引：0
|
作者：
Zhang Xiao-Fei [1 ]
Liu Hui-Hui [2 ]
机构：
[1] Binzhou Coll, Dept Phys & Elect Sci, Binzhou 256600, Shandong, Peoples R China
[2] Henan Univ Sci & Technol, Dept Phys, Luoyang 471003, Peoples R China
来源：
CHINESE PHYSICS LETTERS | 2009年 / 26卷 / 10期
关键词：
HUBBLE-SPACE-TELESCOPE; QUINTOM MODEL; PHANTOM FIELD; CONSTRAINTS; DYNAMICS; CONSEQUENCES; SUPERNOVAE; CONSTANT; EQUATION; UNIVERSE;
D O I：
暂无
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
We construct dark energy models which have high derivative terms. In the framework of a single scalar field model with a higher derivative, the equation of state (EOS) w might have some special character in the evolvement, which states that the universe will evolve in some interesting ways. We study the different kinds of dark energy models, and classify them into several genera by their character in the evolvement.
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页数：4
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